R136a1: The Most Massive and Luminous Blue Hypergiant Star

In summary, R136a1 is a blue hypergiant star with a record-breaking mass of 265 solar masses and luminosity of 8,700,000 times that of the Sun. It is part of the R136 super star cluster in the Large Magellanic Cloud. The star has been losing mass due to being above the Eddington limit and is estimated to have originally held 320 solar masses. Its mass was determined by astronomers using data from the Very Large Telescope and Hubble Space Telescope. In comparison, UY Scuti is currently considered the largest known star.
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R136a1, is a blue hypergiant star

Wikipedia said:
R136a1, is a blue hypergiant star, currently on record as the most massive star known, with an estimated 265 solar masses. The star also holds the record for the most luminous at 8,700,000 times the luminosity of the Sun. Like other hypergiant stars that sit above the Eddington limit, R136a1 has been shedding large portions of its own mass in violent outbursts. It is estimated that at its birth the star held 320 solar masses and has been losing 50 solar masses every few million years. It is a member of R136, a Super star cluster near the center of the 30 Doradus complex (also known as the Tarantula Nebula), in the Large Magellanic Cloud. The mass of the star was determined by astronomers at the University of Sheffield using Very Large Telescope in Chile and data from the Hubble Space Telescope.

Reference:
http://en.wikipedia.org/wiki/R136a1
 
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Related to R136a1: The Most Massive and Luminous Blue Hypergiant Star

1. What is R136a1 and why is it significant?

R136a1 is a massive and luminous blue hypergiant star located in the Large Magellanic Cloud. It is significant because it is currently the most massive and luminous star known in the universe, with a mass estimated to be over 300 times that of the Sun.

2. How was R136a1 discovered?

R136a1 was first identified in 2010 by a team of astronomers using the European Southern Observatory's Very Large Telescope. They were studying a cluster of stars called R136 in the Large Magellanic Cloud and noticed that one star in particular stood out due to its extreme brightness and temperature.

3. What makes R136a1 so massive and luminous?

R136a1's mass and luminosity are believed to be a result of its rapid evolution. It was likely born with a mass of around 250 times that of the Sun, but has since gained additional mass from its surroundings through stellar winds and gravitational interactions with other stars in its cluster.

4. What is the lifespan of R136a1?

Due to its extreme mass and luminosity, R136a1 is expected to have a short lifespan of only a few million years. This is significantly shorter than the Sun's lifespan of about 10 billion years.

5. How does R136a1's mass and luminosity compare to other stars?

R136a1's mass and luminosity are far greater than that of any other known star. It is estimated to be about twice as massive and over 10 million times more luminous than the Sun. This makes it an important object for studying the upper limits of stellar evolution and the formation of massive stars.

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